Systematic surveys of astronomical objects often lead to discoveries, but always provide invaluable information for statistical studies of well-defined samples. They also promote follow-up investigations of individual objects or classes. Surveys using a yet unexplored observing wavelength, a novel technique or a new instrument are of special importance. Significantly improved observing parameters (e.g. sensitivity, angular resolution, monitoring capability) provide new insight into the morphological and physical properties of the objects studied. I give a brief overview of the important Very Long Baseline Interferometry (VLBI) imaging surveys conducted in the past. A list of surveys guides us through the developments up until the present da...
The capabilities of the European very long baseline interferometry (VLBI) network are summarized. Th...
We present the first results from the first Caltech-Jodrell Bank VLBI survey (the CJ1 survey). The C...
The Caltech-Jodrell Bank VLBI surveys of bright extragalactic radio sources north of declination 35°...
Very Long Baseline Interferometry (VLBI) has significant advantages in disentangling active galactic...
Radio observations using the Very Long Baseline Interferometry (VLBI) technique typically have field...
Radio observations using the Very Long Baseline Interferometry (VLBI) technique typically have field...
High angular resolution radio astronomy has undergone several major advancements over the past decad...
For over 20 years, a significant effort has been made to map the milliarcsecond sky with VLBI. The l...
In this paper, I present the likely technological development of VLBI, and its impact on the astrono...
Radio observations using the Very Long Baseline Interferometry (VLBI) technique typically have field...
We report on the first wide-field, very long baseline interferometry (VLBI) survey at 90 cm. The sur...
A systematic very long baseline interferometry (VLBI) sky survey, undertaken to find a suitable set ...
Two large VLBI surveys are currently underway which utilise the snapshot technique pioneered on the ...
Radio observations using the Very Long Baseline Interferometry (VLBI) technique typically have field...
International audienceThe original VLBA Calibrator Surveys (VCS) were a series of 6 VLBA campaigns f...
The capabilities of the European very long baseline interferometry (VLBI) network are summarized. Th...
We present the first results from the first Caltech-Jodrell Bank VLBI survey (the CJ1 survey). The C...
The Caltech-Jodrell Bank VLBI surveys of bright extragalactic radio sources north of declination 35°...
Very Long Baseline Interferometry (VLBI) has significant advantages in disentangling active galactic...
Radio observations using the Very Long Baseline Interferometry (VLBI) technique typically have field...
Radio observations using the Very Long Baseline Interferometry (VLBI) technique typically have field...
High angular resolution radio astronomy has undergone several major advancements over the past decad...
For over 20 years, a significant effort has been made to map the milliarcsecond sky with VLBI. The l...
In this paper, I present the likely technological development of VLBI, and its impact on the astrono...
Radio observations using the Very Long Baseline Interferometry (VLBI) technique typically have field...
We report on the first wide-field, very long baseline interferometry (VLBI) survey at 90 cm. The sur...
A systematic very long baseline interferometry (VLBI) sky survey, undertaken to find a suitable set ...
Two large VLBI surveys are currently underway which utilise the snapshot technique pioneered on the ...
Radio observations using the Very Long Baseline Interferometry (VLBI) technique typically have field...
International audienceThe original VLBA Calibrator Surveys (VCS) were a series of 6 VLBA campaigns f...
The capabilities of the European very long baseline interferometry (VLBI) network are summarized. Th...
We present the first results from the first Caltech-Jodrell Bank VLBI survey (the CJ1 survey). The C...
The Caltech-Jodrell Bank VLBI surveys of bright extragalactic radio sources north of declination 35°...